MAGIC detection of GRB 201216C at z = 1.1

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dc.contributor.authorAbe H
dc.contributor.authorAbe S
dc.contributor.authorAcciari V
dc.contributor.authorAgudo I
dc.contributor.authorAniello T
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dc.contributor.authorCastro-Tirado A
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dc.contributor.authorGarcía López R
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dc.contributor.authorGasparyan S
dc.contributor.authorGaug M
dc.contributor.authorGiesbrecht Paiva J
dc.contributor.authorGiglietto N
dc.contributor.authorGiordano F
dc.contributor.authorGliwny P
dc.contributor.authorGodinović N
dc.contributor.authorGrau R
dc.contributor.authorGreen D
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dc.contributor.authorHütten M
dc.contributor.authorImazawa R
dc.contributor.authorInada T
dc.contributor.authorIotov R
dc.contributor.authorIshio K
dc.contributor.authorJiménez Martínez I
dc.contributor.authorJormanainen J
dc.contributor.authorKerszberg D
dc.contributor.authorKluge G
dc.contributor.authorKobayashi Y
dc.contributor.authorKouch P
dc.contributor.authorKubo H
dc.contributor.authorKushida J
dc.contributor.authorLáinez Lezáun M
dc.contributor.authorLamastra A
dc.contributor.authorLeone F
dc.contributor.authorLindfors E
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dc.contributor.authorLombardi S
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dc.contributor.authorLópez-Coto R
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dc.contributor.authorLópez-Oramas A
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dc.contributor.authorLorini A
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dc.contributor.authorOliveira Fraga B
dc.contributor.authorMajumdar P
dc.contributor.authorMakariev M
dc.contributor.authorManeva G
dc.contributor.authorMang N
dc.contributor.authorManganaro M
dc.contributor.authorMangano S
dc.contributor.authorMannheim K
dc.contributor.authorMariotti M
dc.contributor.authorMartínez M
dc.contributor.authorMas-Aguilar A
dc.contributor.authorMazin D
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dc.contributor.authorMiener T
dc.contributor.authorMiranda J
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dc.contributor.authorMolero González M
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dc.contributor.authorPriyadarshi C
dc.contributor.authorRhode W
dc.contributor.authorRibó M
dc.contributor.authorRico J
dc.contributor.authorRighi C
dc.contributor.authorSahakyan N
dc.contributor.authorSaito T
dc.contributor.authorSatalecka K
dc.contributor.authorSaturni F
dc.contributor.authorSchleicher B
dc.contributor.authorSchmidt K
dc.contributor.authorSchmuckermaier F
dc.contributor.authorSchubert J
dc.contributor.authorSchweizer T
dc.contributor.authorSciaccaluga A
dc.contributor.authorSitarek J
dc.contributor.authorSliusar V
dc.contributor.authorSobczynska D
dc.contributor.authorSpolon A
dc.contributor.authorStamerra A
dc.contributor.authorStrišković J
dc.contributor.authorStrom D
dc.contributor.authorStrzys M
dc.contributor.authorSuda Y
dc.contributor.authorSuutarinen S
dc.contributor.authorTajima H
dc.contributor.authorTakahashi M
dc.contributor.authorTakeishi R
dc.contributor.authorTavecchio F
dc.contributor.authorTemnikov P
dc.contributor.authorTerauchi K
dc.contributor.authorTerzić T
dc.contributor.authorTeshima M
dc.contributor.authorTosti L
dc.contributor.authorTruzzi S
dc.contributor.authorTutone A
dc.contributor.authorUbach S
dc.contributor.authorScherpenberg J
dc.contributor.authorVazquez Acosta M
dc.contributor.authorVentura S
dc.contributor.authorVerguilov V
dc.contributor.authorViale I
dc.contributor.authorVigorito C
dc.contributor.authorVitale V
dc.contributor.authorVovk I
dc.contributor.authorWalter R
dc.contributor.authorWill M
dc.contributor.authorYamamoto T
dc.contributor.authorGomboc A
dc.contributor.authorJordana-Mitjans N
dc.contributor.authorMelandri A
dc.contributor.authorMundell C
dc.contributor.authorShrestha M
dc.contributor.authorSteele I
dc.contributor.organizationfi=Suomen ESO-keskus|en=Finnish Centre for Astronomy with ESO|
dc.contributor.organization-code1.2.246.10.2458963.20.54954054844
dc.contributor.organization-code2609700
dc.converis.publication-id386835415
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/386835415
dc.date.accessioned2025-08-28T00:58:48Z
dc.date.available2025-08-28T00:58:48Z
dc.description.abstract<p>Gamma-ray bursts (GRBs) are explosive transient events occurring at cosmological distances, releasing a large amount of energy as electromagnetic radiation over several energy bands. We report the detection of the long GRB 201216C by the MAGIC telescopes. The source is located at z = 1.1 and thus it is the farthest one detected at very high energies. The emission above 70 GeV of GRB 201216C is modelled together with multiwavelength data within a synchrotron and synchrotron self-Compton (SSC) scenario. We find that SSC can explain the broad-band data well from the optical to the very-high-energy band. For the late-time radio data, a different component is needed to account for the observed emission. Differently from previous GRBs detected in the very-high-energy range, the model for GRB 201216C strongly favours a wind-like medium. The model parameters have values similar to those found in past studies of the afterglows of GRBs detected up to GeV energies. © 2023 The Author(s).<br></p>
dc.format.pagerange5856
dc.format.pagerange5867
dc.identifier.eissn1365-2966
dc.identifier.jour-issn0035-8711
dc.identifier.olddbid206801
dc.identifier.oldhandle10024/189828
dc.identifier.urihttps://www.utupub.fi/handle/11111/48968
dc.identifier.urlhttps://academic.oup.com/mnras/article/527/3/5856/7326795
dc.identifier.urnURN:NBN:fi-fe2025082787476
dc.language.isoen
dc.okm.affiliatedauthorJormanainen, Jenni
dc.okm.affiliatedauthorKouch, Pouya
dc.okm.affiliatedauthorLindfors, Elina
dc.okm.affiliatedauthorNilsson, Kari
dc.okm.affiliatedauthorSatalecka, Konstancja
dc.okm.affiliatedauthorSuutarinen, Sofia
dc.okm.discipline114 Physical sciencesen_GB
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline114 Fysiikkafi_FI
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherOxford University Press
dc.publisher.countryUnited Kingdomen_GB
dc.publisher.countryBritanniafi_FI
dc.publisher.country-codeGB
dc.relation.doi10.1093/mnras/stad2958
dc.relation.ispartofjournalMonthly Notices of the Royal Astronomical Society
dc.relation.issue3
dc.relation.volume527
dc.source.identifierhttps://www.utupub.fi/handle/10024/189828
dc.titleMAGIC detection of GRB 201216C at z = 1.1
dc.year.issued2024

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